1/ π’ This is an image mosaic of 18 randomly organised dots of starlight, the product of #Webb 's unaligned mirror segments all reflecting light from the same star back at Webb's secondary mirror and into #NIRCam's detectors. Thread π with a surprise at the end!
2/ The mosaic was created by pointing the telescope at a bright, isolated star in the constellation Ursa Major known as HD 84406, chosen specifically because it's easily identifiable and not crowded by other stars of similar brightness, which helps to reduce background confusion
3/ Each dot within the mosaic is labeled by the corresponding primary mirror segment that captured it. These initial results closely match expectations and simulations.
4/ During the image capturing process that began on 2 February #Webb was repointed to 156 different positions around the predicted location of the star and generated 1,560 images using NIRCamβs 10 detectors, amounting to 54 gigabytes of raw data.
5/ The entire process lasted nearly 25 hours, but the observatory was able to locate the target star π― in each of its mirror segments within the first six hours and 16 exposures.
6/ These images were then stitched together to produce a single, large mosaic that captures the signature of each primary mirror segment in one frame. The images shown above are only a centre portion of that larger mosaic, a huge image with over 2 billion pixels.
7/ This activity determined the post-deployment alignment positions of every mirror segment, which is the critical first step in bringing the entire observatory into a functional alignment for scientific operations.
8/ What looks like a simple image of blurry starlight now becomes the foundation to align and focus the telescope in order for #Webb to deliver unprecedented views of the universe this summer. #WebbSeesFarther
9/ Over the next month or so, the team will gradually adjust the mirror segments until the 18 images become a single star βοΈβ‘οΈβοΈβ¬ οΈβοΈ
10/ Moving forward, #Webbβs images will only become clearer, more detail-laden & more intricate as its other 3 instruments arrive at their intended operating temperatures & begin capturing data. The first scientific images are expected to be delivered to the world in the summer.
11/ But wait, there's more! We also have #Webb's first "selfie" π€³ This image was created using a specialised pupil imaging lens inside of the #NIRCam instrument that was designed to take images of the primary mirror segments instead of images of space.
π· NASA
12. This configuration is not used during scientific operations, it's strictly for engineering & alignment purposes. The bright segment βοΈwas pointed at a bright star, while the others arenβt currently in the same alignment. Full blog here: blogs.nasa.gov/webb/2022/02/1β¦
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Taking #Webb's temperature π‘οΈ 5 new temperature monitoring points have been added to the NASA website to track cooling and status of the instruments during the post L2 arrival commissioning process. Let's have a look at them π
1/ Temperature control is a vital aspect of #Webb 's design, engineering and operations. On the page you can see 2 "hot side" and 2 "cold side" temperatures and a set of bellweather instrument temperatures
2/ The instruments are located within the Integrated Science Instrument Module and the Fine Steering Mirror is located within the protrusion in the center of the primary mirror
Some of you asked recently why are #Webb's mirrors hexagonal? Thread π
π· NASA/Chris Gunn
1/ The hexagonal shape enables a roughly circular, segmented mirror with "high filling factor and six-fold symmetry." High filling factor just means the segments fit together without gaps, which would not be the case if the segments were circular
2/ Symmetry is good because only 3 different optical prescriptions (A, B and C) are needed for 18 segments, 6 of each as seen below π· NASA
As #Webb is going through the focusing of its mirrors, let's look into what this process entails. #WebbSeesFarther π
1/ #Webb's 18 hexagonal mirrors have already been unfolded a while back, but now it's time for a more precise alignment so they point in exactly the same direction π― and deliver sharp images.
π· NASA/Chris Gunn
2/ These corrections are made through a process called γ°οΈ wavefront sensing and control, which senses and corrects any errors in the telescope's optics, aligning the mirrors to within tens of nanometres
1/ While we wait for news on L2 orbit insertion, we've got some facts for you on #Webb's orbit π
2/ Unlike @Hubble_Space#Webb will not be in orbit around the Earth, but will orbit the Sun, 1.5 million km away from the π at what is called the second Lagrange point or L2.
3/ This orbit lets the telescope stay in line with the Earth as it moves around the Sun. This allows the satellite's large sunshield to protect the telescope from the light and heat of the Sun, Earth and Moon.
1/ The Mid-InfraRed Instrument #MIRI is one of 4 instruments on the James #Webb Space Telescope. The only mid-infrared instrument in its instrument suite. #WebbSeesFarther
π· NASA/ Chris Gunn
2/ Thanks to state-of-the-art instrument design and components, it will deliver mid-infrared images and spectra with an unprecedented combination of sharpness and sensitivity. #WebbSeesFarther
3/ #MIRI will be capable of penetrating thick layers of dust obscuring regions of intense star birth. It will see the first generations of galaxies to form after the #BigBang, and it will study sites of new planet formation and the composition of the interstellar medium.